S/2004 S 4
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Discovery | |
---|---|
Discovered by | Joseph Spitale / Cassini Imaging Science Team.[1] |
Discovered on | 21 June 2004 |
Orbital characteristics | |
Semimajor axis | ~140,100 km.[2] |
Eccentricity | unknown, small |
Orbital period | ~0.618 d [2] |
Inclination | unknown, small |
Is a satellite of | Saturn |
Physical characteristics | |
Mean diameter | 3-5 km |
Rotation period | probably synchronous |
Axial tilt | unknown |
Albedo | unknown |
Atmosphere | none |
S/2004 S 4 is the provisional designation of an unconfirmed object seen orbiting Saturn within the inner strand of the F ring on 21 June 2004. It was spotted while J. N. Spitale was trying to confirm the orbit of another provisional object, S/2004 S 3 that was seen 5 hours earlier just exterior to the F ring.[1] The announcement was made on September 9, 2004.[3]
Despite later attempts to recover it, it has not been reliably sighted since. Notably, an imaging sequence covering an entire orbital period at 4 km resolution taken on 15 November 2004 failed to recover the object. This suggests that it was a temporary clump of material that had disappeared by that time.[4]
An interpretation where S3 and S4 are or were a single object on a F-ring crossing orbit is also possible.[3] Such an object might also be orbiting at a slightly different inclination to the F ring, thereby not actually passing through the ring material despite being seen both radially inward and outward of it.
If a solid object after all, S/2004 S 4 would be 3−5 km in diameter based on brightness.
[edit] References
- ^ a b Martinez, C.; Ormrod, G.; and Finn, H.; Cassini-Huygens Press Releases: Cassini Discovers Ring and One, Possibly Two, Objects at Saturn September 9, 2004
- ^ a b PGJ Astronomie webpage (Gilbert Javaux) Note that the F ring is centered at ~140,180 km
- ^ a b IAUC 8401: S/2004 S 3, S/2004 S 4, and R/2004 S 1 2004 September 9 (discovery)
- ^ Spitale, J. N.; et al. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal 132: 692. doi: .
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